The main goal of this thesis is to investigate the physical conditions of the star-forming environment in stellar clusters, especially for the formation of low-mass cluster members. Embedded, young, and intermediate-mass stellar clusters around Herbig . Ae/Be stars are
sampled. Mid- and near-infrared observations identifying young stars and millimeter
interferometric observations probing dense molecular gas and dust continuum are presented.
These observations are used to reveal the large-scale young stellar population around the vicinity
where the sampled clusters form, probe the physical conditions of dense molecular clumps which
are capable of forming individual low-mass cluster members, and examine the influence of the
most massive star in the cluster on its siblings and natal cluster-forming cloud. This study shows
that stars within the cluster tend to seem younger than those outside the cluster, suggesting a
higher and continuous star-forming rate within the cluster than outside, or massive stars are
initiated later than low-mass star within the same cloud. A thorough investigation of young stars
and dense gas toward the MWC·l080 cluster further suggests a domination of the.most massive
star in the cluster on both the natal cloud dispersal and its low-mass cluster members. As active
outflows and winds from the Herbig Ae/Be stars increase the non-thermal motion in the cloud,
low-mass cluster members are formed within denser and more. turbulent cores, than isolated low-mass
star-forming cores. In addition, the strong gas dispersal from the Herbig Ae/Be stars also
helps the removal of the circumstellar material around nearby low-mass stars. This makes these
low-mass cluster members appear older. In summary, this thesis provides the observational
evidence showing how the most massive star in the cluster affects the formation and evolution of
low-mass cluster members and the physical conditions of star formation in the cluster.

Issue Date:

2008

Publisher:

Department of Astronomy. College of Liberal Arts and Science. The University of Illinois at Urbana-Champaign.